............. MAKEE: Keck ESI Reduction .......... Tue Nov 7 13:03:37 2000 MAKEE VERSION= 3.2.0 : October 2000 OBJECT: 0 2231 0 4095 ./esi0076.fits Object 0.75 STAR: 0 2231 0 4095 ./esi0065.fits Object 0.75 FLAT: 0 2231 0 4095 ./esi0058.fits IntFlat 0.75 ARC: 0 2231 0 4095 ./esi0083.fits Line 0.75 ARC2: 0 2231 0 4095 ./esi0084.fits Line 0.75 Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 76 0324.9-0456 Expos= 3000s Object=SDSSp0324-0457 Object to extract: SDSSp0324-0457 0322-0107 00/10/24 13:28:33 76 3000s Binning: 1x1 File: esi0076.fits Mode= 1 Extract all orders. Masking file: MaskESI_1x1_2.dat Bias file: /users/tab/makee///biasESI_1x1_2amp.fits ............ Reading bias : /users/tab/makee///biasESI_1x1_2amp.fits Using 1 dimensional processed bias image. Bias image observation date: 2000-10-21 ............ Reading flat : ./esi0058.fits Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 58 0517.2+0003 Expos= 6s Object=IntFlat NOTE: Using special interpolation for ESI. Subtracting baseline ( 2072 --> 2151 ) from data ( 24 --> 1047 ). Subtracting baseline ( 2152 --> 2231 ) from data ( 1048 --> 2071 ). Rotating ESI image by 90 degrees... Flipping ESI image in columns... Prepix: 12 Postpix: 80 Original Window: cols= 0 2048 rows= 0 4096 New Clipped Window: cols= 0 4094 rows= 0 2045 Subtracting bias from image... ............ Estimate slit length from flat field... Estimate for slit length = 127.390 Saving flat image... junk-flat_0973631028000076001.fits ............ Reading star : ./esi0065.fits Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 65 2151.1+2851 Expos= 100s Object=BD+28 4211 NOTE: Using special interpolation for ESI. Subtracting baseline ( 2072 --> 2151 ) from data ( 24 --> 1047 ). Subtracting baseline ( 2152 --> 2231 ) from data ( 1048 --> 2071 ). Rotating ESI image by 90 degrees... Flipping ESI image in columns... Prepix: 12 Postpix: 80 Original Window: cols= 0 2048 rows= 0 4096 New Clipped Window: cols= 0 4094 rows= 0 2045 Subtracting bias from image... Finding and fitting order traces... Writing PostScript plot file: trace-065.ps NOTE: EETO: EON= 1 High= 2.097 WRMS= 0.303 WPPD= 0.372 NREJ= 32 NOTE: EETO: EON= 2 High= 1.341 WRMS= 0.197 WPPD= 0.301 NREJ= 48 NOTE: EETO: EON= 3 High= 0.974 WRMS= 0.144 WPPD= 0.271 NREJ= 43 NOTE: EETO: EON= 4 High= 0.757 WRMS= 0.109 WPPD= 0.245 NREJ= 58 NOTE: EETO: EON= 5 High= 0.490 WRMS= 0.072 WPPD= 0.203 NREJ= 104 NOTE: EETO: EON= 6 High= 0.305 WRMS= 0.044 WPPD= 0.183 NREJ= 75 NOTE: EETO: EON= 7 High= 0.212 WRMS= 0.032 WPPD= 0.177 NREJ= 20 NOTE: EETO: EON= 8 High= 0.189 WRMS= 0.034 WPPD= 0.179 NREJ= 7 NOTE: EETO: EON= 9 High= 0.386 WRMS= 0.058 WPPD= 0.192 NREJ= 2 NOTE: EETO: EON= 10 High= 4.335 WRMS= 0.767 WPPD= 0.714 NREJ= 0 Number of echelle orders = 10 Recovering flat image... junk-flat_0973631028000076001.fits Estimating background limits... NOTE: Background between widely separated orders: 3.33664E+02 NOTE: EEFB: EON= 1 Slit Edge Lower= 83.6 Upper= -76.2 Width= 159.8 NOTE: EEFB: EON= 2 Slit Edge Lower= 78.3 Upper= -73.7 Width= 152.0 NOTE: EEFB: EON= 3 Slit Edge Lower= 74.3 Upper= -71.3 Width= 145.6 NOTE: EEFB: EON= 4 Slit Edge Lower= 70.7 Upper= -68.7 Width= 139.4 NOTE: EEFB: EON= 5 Slit Edge Lower= 67.7 Upper= -66.5 Width= 134.2 NOTE: EEFB: EON= 6 Slit Edge Lower= 64.9 Upper= -64.5 Width= 129.4 NOTE: EEFB: EON= 7 Slit Edge Lower= 62.6 Upper= -62.9 Width= 125.5 NOTE: EEFB: EON= 8 Slit Edge Lower= 60.4 Upper= -61.2 Width= 121.6 NOTE: EEFB: EON= 9 Slit Edge Lower= 58.4 Upper= -59.5 Width= 117.9 NOTE: EEFB: EON= 10 Slit Edge Lower= 56.5 Upper= -57.8 Width= 114.3 EEFB: Fitting background lower offsets. EEFB: Fitting background upper offsets. Flat field scale factor= 6.888359E+03 Saving flat image... junk-flat_0973631028000076001.fits ............ Reading object : ./esi0076.fits Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 76 0324.9-0456 Expos= 3000s Object=SDSSp0324-0457 NOTE: Using special interpolation for ESI. Subtracting baseline ( 2072 --> 2151 ) from data ( 24 --> 1047 ). Subtracting baseline ( 2152 --> 2231 ) from data ( 1048 --> 2071 ). Rotating ESI image by 90 degrees... Flipping ESI image in columns... Prepix: 12 Postpix: 80 Original Window: cols= 0 2048 rows= 0 4096 New Clipped Window: cols= 0 4094 rows= 0 2045 Subtracting bias from image... Observation number= 76 UT date = 24Oct00 Masking bad regions... NOTE: Object x,y binning is 1 x 1 . Recovering flat image... junk-flat_0973631028000076001.fits Dividing object by flat field... Determine object profile and boundaries... Writing FITS profile file: profiles-076.fits Writing PostScript plot file: profiles-076.ps slit width, neo, eperdn, ronoise, pse_mode = 127.39 10 0.500 2.700 1 ****************************** Extracting echelle order number 1 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00271 Sky Pixels Masked (primary,adjacent,additional): 729 326 376 Sky areas ratio: 0.737. Sky polynomial order: 1. Object Pixels Masked (high,low): 202 2 PSE_ObjSum: Had to deal with 219 masked pixels. ****************************** Extracting echelle order number 2 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00275 Sky Pixels Masked (primary,adjacent,additional): 972 485 917 Sky areas ratio: 0.762. Sky polynomial order: 1. Object Pixels Masked (high,low): 167 8 PSE_ObjSum: Had to deal with 189 masked pixels. ****************************** Extracting echelle order number 3 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00345 Sky Pixels Masked (primary,adjacent,additional): 1110 742 1065 Sky areas ratio: 0.787. Sky polynomial order: 1. Object Pixels Masked (high,low): 403 0 PSE_ObjSum: Had to deal with 432 masked pixels. ****************************** Extracting echelle order number 4 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00222 Sky Pixels Masked (primary,adjacent,additional): 669 450 1314 19 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.813. Sky polynomial order: 1. Object Pixels Masked (high,low): 177 0 PSE_ObjSum: Had to deal with 190 masked pixels. ****************************** Extracting echelle order number 5 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00236 Sky Pixels Masked (primary,adjacent,additional): 691 458 1673 118 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.840. Sky polynomial order: 1. Object Pixels Masked (high,low): 253 0 PSE_ObjSum: Had to deal with 288 masked pixels. ****************************** Extracting echelle order number 6 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00258 Sky Pixels Masked (primary,adjacent,additional): 712 415 1371 427 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.865. Sky polynomial order: 1. Object Pixels Masked (high,low): 282 0 PSE_ObjSum: Had to deal with 318 masked pixels. ****************************** Extracting echelle order number 7 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00209 Sky Pixels Masked (primary,adjacent,additional): 613 352 1165 543 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.890. Sky polynomial order: 1. Object Pixels Masked (high,low): 270 3 PSE_ObjSum: Had to deal with 304 masked pixels. ****************************** Extracting echelle order number 8 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00308 Sky Pixels Masked (primary,adjacent,additional): 1216 516 856 1162 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.912. Sky polynomial order: 1. Object Pixels Masked (high,low): 145 13 PSE_ObjSum: Had to deal with 138 masked pixels. ****************************** Extracting echelle order number 9 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00290 Sky Pixels Masked (primary,adjacent,additional): 1573 425 732 1421 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.931. Sky polynomial order: 1. Object Pixels Masked (high,low): 355 7 PSE_ObjSum: Had to deal with 379 masked pixels. ****************************** Extracting echelle order number 10 of 10 Cosmic Ray Fraction: expected= 0.00225 actual= 0.00226 Sky Pixels Masked (primary,adjacent,additional): 996 318 1398 1218 columns affected by nearby night sky lines during SkyFit. Sky areas ratio: 0.946. Sky polynomial order: 1. Object Pixels Masked (high,low): 389 4 PSE_ObjSum: Had to deal with 395 masked pixels. Writing : Flux-076.fits Writing : Var-076.fits Writing : Sky-076.fits Writing : Sum-076.fits Tue Nov 7 13:08:06 2000 ..... Extracting Flat Field Spectrum ........... ............ Reading object : ./esi0058.fits Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 58 0517.2+0003 Expos= 6s Object=IntFlat NOTE: Using special interpolation for ESI. Subtracting baseline ( 2072 --> 2151 ) from data ( 24 --> 1047 ). Subtracting baseline ( 2152 --> 2231 ) from data ( 1048 --> 2071 ). Rotating ESI image by 90 degrees... Flipping ESI image in columns... Prepix: 12 Postpix: 80 Original Window: cols= 0 2048 rows= 0 4096 New Clipped Window: cols= 0 4094 rows= 0 2045 Subtracting bias from image... Observation number= 58 UT date = 23Oct00 Masking bad regions... NOTE: Object x,y binning is 1 x 1 . Recovering flat image... junk-flat_0973631028000076001.fits Dividing object by flat field... slit width, neo, eperdn, ronoise, pse_mode = 127.39 10 0.500 2.700 4 Extracting whole slit spectrum... ****************************** Extracting echelle order number 1 of 10 ****************************** Extracting echelle order number 2 of 10 ****************************** Extracting echelle order number 3 of 10 ****************************** Extracting echelle order number 4 of 10 ****************************** Extracting echelle order number 5 of 10 ****************************** Extracting echelle order number 6 of 10 ****************************** Extracting echelle order number 7 of 10 ****************************** Extracting echelle order number 8 of 10 ****************************** Extracting echelle order number 9 of 10 ****************************** Extracting echelle order number 10 of 10 Writing : Flat-058.fits Tue Nov 7 13:08:22 2000 ..... Extracting Arc Lamp Spectrum ........... ............ Reading object : ./esi0083.fits Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 83 0517.2+0003 Expos= 300s Object=CuAr NOTE: Using special interpolation for ESI. Subtracting baseline ( 2072 --> 2151 ) from data ( 24 --> 1047 ). Subtracting baseline ( 2152 --> 2231 ) from data ( 1048 --> 2071 ). Rotating ESI image by 90 degrees... Flipping ESI image in columns... Prepix: 12 Postpix: 80 Original Window: cols= 0 2048 rows= 0 4096 New Clipped Window: cols= 0 4094 rows= 0 2045 Subtracting bias from image... Observation number= 83 UT date = 24Oct00 Masking bad regions... NOTE: Object x,y binning is 1 x 1 . Recovering flat image... junk-flat_0973631028000076001.fits Dividing object by flat field... slit width, neo, eperdn, ronoise, pse_mode = 127.39 10 0.500 2.700 4 Extracting whole slit spectrum... ****************************** Extracting echelle order number 1 of 10 ****************************** Extracting echelle order number 2 of 10 ****************************** Extracting echelle order number 3 of 10 ****************************** Extracting echelle order number 4 of 10 ****************************** Extracting echelle order number 5 of 10 ****************************** Extracting echelle order number 6 of 10 ****************************** Extracting echelle order number 7 of 10 ****************************** Extracting echelle order number 8 of 10 ****************************** Extracting echelle order number 9 of 10 ****************************** Extracting echelle order number 10 of 10 Writing : Arc-083.fits Tue Nov 7 13:08:38 2000 ..... Extracting Second Arc Lamp Spectrum ........... ............ Reading object : ./esi0084.fits Setting EPERDN = 0.5000 Setting RONOISE = 2.7000 Column binning= 1 Row binning= 1 Frame#= 84 0517.2+0003 Expos= 4s Object=Hg+Xe NOTE: Using special interpolation for ESI. Subtracting baseline ( 2072 --> 2151 ) from data ( 24 --> 1047 ). Subtracting baseline ( 2152 --> 2231 ) from data ( 1048 --> 2071 ). Rotating ESI image by 90 degrees... Flipping ESI image in columns... Prepix: 12 Postpix: 80 Original Window: cols= 0 2048 rows= 0 4096 New Clipped Window: cols= 0 4094 rows= 0 2045 Subtracting bias from image... Observation number= 84 UT date = 24Oct00 Masking bad regions... NOTE: Object x,y binning is 1 x 1 . Recovering flat image... junk-flat_0973631028000076001.fits Dividing object by flat field... slit width, neo, eperdn, ronoise, pse_mode = 127.39 10 0.500 2.700 4 Extracting whole slit spectrum... ****************************** Extracting echelle order number 1 of 10 ****************************** Extracting echelle order number 2 of 10 ****************************** Extracting echelle order number 3 of 10 ****************************** Extracting echelle order number 4 of 10 ****************************** Extracting echelle order number 5 of 10 ****************************** Extracting echelle order number 6 of 10 ****************************** Extracting echelle order number 7 of 10 ****************************** Extracting echelle order number 8 of 10 ****************************** Extracting echelle order number 9 of 10 ****************************** Extracting echelle order number 10 of 10 Writing : Arc-084.fits Tue Nov 7 13:08:55 2000 Compute wavelength scale for Arc-083.fits ... and include Arc-084.fits arc2obj Arc-083.fits Flux-076.fits bracket=Arc-084.fits arcmode=0 -sky -var ps=Flux-076-skyshift.ps -sum Reading: Arc-083.fits Arc file= Arc-083.fits NOTE: Skylines from: /users/tab/makee////SkyLineDataBase/sky.results.ESI Reading: Arc-084.fits Reading: Flux-076.fits Second file= Flux-076.fits Reading: Var-076.fits Reading: Sum-076.fits Reading: Sky-076.fits *****Night sky line shift results: # row wavelength peak pix.shft weight 1 5 5589.128 27.6 -0.05 0.28 2 5 5889.953 482.4 -0.17 1.00 3 5 5895.923 301.1 -0.17 1.00 4 5 5915.301 60.8 -0.15 0.61 5 5 5924.723 34.5 -0.12 0.34 6 5 5932.862 47.2 -0.13 0.47 7 5 5945.932 27.4 -0.09 0.27 8 5 5953.420 39.7 -0.13 0.40 9 5 5970.278 32.6 -0.05 0.33 10 6 5889.953 482.4 -0.10 1.00 11 6 5895.923 301.1 -0.10 1.00 12 6 5915.301 60.8 -0.05 0.61 13 6 5924.723 34.5 -0.17 0.34 14 6 5932.862 47.2 -0.04 0.47 15 6 5945.932 27.4 -0.05 0.27 16 6 5953.420 39.7 -0.03 0.40 17 6 5970.278 32.6 -0.15 0.33 18 6 6257.961 69.7 -0.48 0.70 19 6 6287.434 62.0 -0.19 0.62 20 6 6297.903 31.0 -0.14 0.31 21 6 6300.304 673.7 -0.24 1.00 22 6 6477.910 38.0 -0.18 0.38 23 6 6498.729 107.4 -0.30 1.00 24 6 6504.995 27.6 -0.14 0.28 25 6 6522.425 62.2 -0.04 0.62 26 6 6544.022 59.8 0.18 0.60 27 6 6553.617 63.2 0.09 0.63 28 7 6257.961 69.7 -0.46 0.70 29 7 6287.434 62.0 0.04 0.62 30 7 6297.903 31.0 -0.03 0.31 31 7 6300.304 673.7 0.00 1.00 32 7 6477.910 38.0 -0.06 0.38 33 7 6498.729 107.4 -0.26 1.00 34 7 6504.995 27.6 -0.08 0.28 35 7 6522.425 62.2 -0.01 0.62 36 7 6544.022 59.8 0.03 0.60 37 7 6553.617 63.2 -0.13 0.63 38 7 6568.779 62.0 -0.08 0.62 39 7 6596.643 37.6 -0.18 0.38 40 7 6841.945 40.7 -0.37 0.41 41 7 6863.955 255.9 -0.50 1.00 42 7 6870.994 29.4 -0.01 0.29 43 7 6900.833 63.8 -0.36 0.64 44 7 6969.930 101.8 -0.31 1.00 45 7 7253.127 109.6 -0.24 1.00 46 7 7276.405 492.0 -0.56 1.00 47 7 7284.439 159.0 -0.14 1.00 48 8 7253.127 109.6 0.12 1.00 49 8 7276.405 492.0 -0.38 1.00 50 8 7284.439 159.0 0.08 1.00 51 8 7316.282 379.4 -0.09 1.00 52 8 7329.148 252.3 -0.01 1.00 53 8 7340.885 424.4 -0.09 1.00 54 8 7358.659 290.6 -0.10 1.00 55 8 7392.198 308.4 -0.14 1.00 56 8 7429.781 134.5 -0.13 1.00 57 8 7530.713 336.9 -0.23 1.00 58 8 7557.492 240.3 -0.07 1.00 59 8 7571.746 443.1 -0.05 1.00 60 8 7586.093 238.1 -0.11 1.00 61 8 7759.996 410.1 -0.08 1.00 62 8 7808.467 526.5 -0.04 1.00 63 8 7821.503 1119.7 -0.14 1.00 64 8 7841.266 844.4 -0.12 1.00 65 8 7860.658 1044.8 -0.19 1.00 66 8 7870.730 1196.6 -0.06 1.00 67 8 8014.059 1149.3 -0.21 1.00 68 8 8052.020 1072.3 -0.46 1.00 69 9 8014.059 1149.3 0.06 1.00 70 9 8052.020 1072.3 -0.30 1.00 71 9 8288.603 1786.7 -0.23 1.00 72 9 8298.896 1956.7 -0.13 1.00 73 9 8382.392 1366.9 -0.30 1.00 74 9 8493.389 932.7 0.10 1.00 75 9 8903.114 1558.9 -0.05 1.00 76 9 8919.634 2112.7 -0.09 1.00 Skyline shift= -0.1454 +/- 0.1459 Npt= 76 NRej= 0 Writing to device: Flux-076-skyshift.ps/PS Applying skyline shift of -0.1454 pixels to arclamp scale. Sky Shift used= -0.1454 measured= -0.1454 RMS= 0.1459 #Pt= 76 Heliocentric velocity correction (km/s) = 7.7047 Air to vacuum correction applied... Heliocentric velocity correction applied... Over-writing file: Flux-076.fits Over-writing file: Sum-076.fits Over-writing file: Sky-076.fits Writing file: Err-076.fits arc2obj: All done. ..................................................... arc2arc Flux-076.fits Sum-076.fits pxsh=0 First file= Flux-076.fits Second file= Sum-076.fits Shift in pixels= 0.000000 Zero shift, no refitting necessary. arc2arc: All done. opim mul Flux-076.fits Flat-058.fits DN-076.fits -clobber Writing file : DN-076.fits opim div DN-076.fits const=+6.8883594E+03 -clobber Writing file : DN-076.fits spim0 DN-076.fits min=0. bin=2 ps=DN-076.ps Output is in : DN-076.ps opim div Flux-076.fits Err-076.fits s2n-076.fits -clobber Writing file : s2n-076.fits opim min s2n-076.fits const=0. -clobber Writing file : s2n-076.fits spim0 s2n-076.fits min=0. bin=2 ps=s2n-076.ps Output is in : s2n-076.ps spim0 Flux-076.fits minp=-0.08 bin=2 ps=Flux-076.ps Output is in : Flux-076.ps NOTE: spectrum plot binning factor is 2 pixels. rhh Flux-076.fits -wave 76 Flux-076 24Oct00 13:28 Ec:Obje 0.75 1x1 3000s SDSSp0324-0457 (Fl Tue Nov 7 13:08:57 2000 makee: All done.